All-inclusive interacting dark sector cosmologies

Abstract

In this paper we explore possible extensions of Interacting Dark Energy cosmologies, where Dark Energy and Dark Matter interact non-gravitationally with one another. In particular, we focus on the neutrino sector, analyzing the effect of both neutrino masses and the effective number of neutrino species. We consider the Planck 2018 legacy release data combined with several other cosmological probes, finding no evidence for new physics in the dark radiation sector. The current neutrino constraints from cosmology should be therefore regarded as robust, as they are not strongly dependent on the dark sector physics, once all the available observations are combined. Namely, we find a total neutrino mass $M_{\nu }<0.15$ eV and a number of effective relativistic degrees of freedom of $N_{\mathrm{eff}}=3.03_{-0.33}^{+0.33}$, both at 95\% CL, which are close to those obtained within the $\Lambda$CDM cosmology, $M_{\nu }<0.12$ eV and $N_{\mathrm{eff}}=3.00_{-0.35}^{+0.36}$ for the same data combination.

arXiv comment15 pages, 8 Tables, 8 captioned Figures, accepted for publication in PRD

References in corpus (66)

• Planck 2015 results. XIII. Cosmological parameters
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• Efficient Computation of CMB anisotropies in closed FRW models
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• Relic neutrino decoupling including flavour oscillations
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
• Non-minimal dark sector physics and cosmological tensions
• Gravitational Lensing Analysis of the Kilo Degree Survey
• Can interacting dark energy solve the $H_0$ tension?
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey - Imaging Data and Catalogue Products
• Large-scale instability in interacting dark energy and dark matter fluids
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Relic neutrino decoupling with flavour oscillations revisited
• Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data
• CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics
• Cosmologies with Energy Exchange
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z)\ge -1$ are tighter than those obtained in $\Lambda$CDM
• Interactions in Scalar Field Cosmology
• Echo of interactions in the dark sector
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• Dark coupling
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Interacting Dark Energy -- constraints and degeneracies
• Dark sector interaction: a remedy of the tensions between CMB and LSS data
• Calibration of weak-lensing shear in the Kilo-Degree Survey
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Constraints on the interacting vacuum -- geodesic CDM scenario
• Effective Theory of Interacting Dark Energy
• Adiabatic initial conditions for perturbations in interacting dark energy models
• An analytic model for interacting dark energy and its observational constraints
• A new interacting two fluid model and its consequences
• Field theoretic interpretations of interacting dark energy scenarios and recent observations
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Galaxy clustering, photometric redshifts and diagnosis of systematics in the DES Science Verification data
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Dark Coupling and Gauge Invariance
• Testing coupled dark energy with large scale structure observation
• A model with interaction of dark components and recent observational data
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• In search of the dark matter dark energy interaction: a kinematic approach
• Dynamics of nonlinear interacting dark energy models
• Cosmological constraints on an exponential interaction in the dark sector
• Observational constraints on dark matter-dark energy scattering cross section
• Dynamics and cosmological evolution in Λ-varying cosmology
• Large-scale (in-) stability Analysis of an Exactly Solved Coupled Dark-Energy Model
• Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Higher neutrino mass allowed if Cold Dark Matter and Dark Energy are coupled

Cited by in corpus (57)

• In the Realm of the Hubble tension $-$ a Review of Solutions
• Challenges for $\Lambda$CDM: An update
• Cosmology Intertwined II: The Hubble Constant Tension
• Non-minimal dark sector physics and cosmological tensions
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Cosmological solutions and growth index of matter perturbations in $f(Q)$ gravity
• A combined analysis of the $H_0$ late time direct measurements and the impact on the Dark Energy sector
• On the most constraining cosmological neutrino mass bounds
• Cosmological parameter analyses using transversal BAO data
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• Interacting Dark Energy in a closed universe
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Dark sector interaction and the supernova absolute magnitude tension
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• New constraints on interacting dark energy from DESI DR2 BAO observations
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Soundness of Dark Energy properties
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Late time interacting cosmologies and the Hubble constant tension
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• A double take on early and interacting dark energy from JWST
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• A fake Interacting Dark Energy detection?
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Addressing $H_0$ tension with emergent dark radiation in unitary gravity
• Dynamical Dark sectors and Neutrino masses and abundances
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Model marginalized constraints on neutrino properties from cosmology
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Growth of matter perturbations in the extended viscous dark energy models
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• An absolute $\nu$ mass measurement with the DUNE experiment
• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Thomson scattering: One rate to rule them all
• Hubble distancing: Focusing on distance measurements in cosmology
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Do we need wavelets in the late Universe?
• Interacting phantom dark energy: new accelerating scaling attractors
• Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• $\Lambda$CDM as a Noether Symmetry in Cosmology
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Probing Interacting Dark Sector with the next generation of gravitational-wave detectors
• Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
• Studies on dark energy evolution
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Crunching, Bouncing, and Cyclical Cosmologies from Dark Sector Interactions
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension